MOND, based on a modifications of Newton's law for small accelerations, describes the rotation curves of stars in most galaxies, especially the outer stars.
Has MOND been tested for the stars in our own galaxy, the Milky Way? Is there any publication on this topic?
It appears that Does MOND make good predictions? does not answer this question, because it is about other galaxies; it does not discuss the Milky Way at all. This question is about rotation curves of the stars in the Milky Way only - not about other stars.
The challenge is different, because one has to measure many different stars at many different positions in the sky, and then deduce the rotation curve.